Relative frequencies of supernovae versus properties of spiral hosts

Preprint English OPEN
Hakobyan, A. A. ; Nazaryan, T. A. ; Adibekyan, V. Zh. ; Petrosian, A. R. ; Aramyan, L. S. ; Kunth, D. ; Mamon, G. A. ; de Lapparent, V. ; Bertin, E. ; Gomes, J. M. ; Turatto, M. (2013)
  • Related identifiers: doi: 10.1017/S1743921314004220
  • Subject: Astrophysics - Astrophysics of Galaxies | Astrophysics - Cosmology and Nongalactic Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Solar and Stellar Astrophysics

In this work, we present an analysis of SNe number ratios in spiral galaxies with different morphological subtypes, luminosities, sSFR, and metallicities, to provide important information about the physical properties of the progenitor populations.
  • References (1)

    Boissier, S., & Prantzos, N. 2009, A&A, 503, 137 Eldridge, J. J., Izzard, R. G., & Tout, C. A. 2008, MNRAS, 384, 1109 Hakobyan, A. A., Adibekyan, V. Z., Aramyan, L. S., et al. 2012, A&A, 544, A81 Hakobyan, A. A., Nazaryan, T. A., Adibekyan, V. Z., et al. 2014, in preparation

  • Metrics
    No metrics available
Share - Bookmark